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High-Dispersion Spectroscopy of the Brightest Emission-Line Stars of the Magellanic Clouds

Published online by Cambridge University Press:  04 August 2017

O. Stahl ,
B. Wolf ,
M. de Groot  and
C. Leitherer
O. Stahl
Affiliation:
Landessternwarte, Königstuhl, Germany
B. Wolf
Affiliation:
Landessternwarte, Königstuhl, Germany
M. de Groot
Affiliation:
Armagh Observatory, Northern Ireland
C. Leitherer
Affiliation:
Landessternwarte, Königstuhl, Germany

Extract

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We present an atlas of high dispersion spectra of 24 of the brightest peculiar emission-line stars of the Magellanic Clouds.

Our spectra cover the wavelength range from 3600 to 4900 Å. They have been obtained from 1970 to 1984 with the coudé spectrograph of the ESO 1.52 m telescope at La Silla, Chile. The spectral resolution is 0.4 Å for most of the spectra and 0.2 Å for the very brightest stars. Up to 11 spectra are available for one star. In addition, we have done UBVRIJHK(LM) photometry at several epochs of all stars of our sample.

Type
Poster Papers 2
Information
Symposium - International Astronomical Union , Volume 116: Luminous Stars and Associations in Galaxies , 1986 , pp. 247 - 248
Copyright
Copyright © Reidel 1986